Home
Astronomy research
Software instruments
Stellar equation of states
EOS with ionization
EOS for supernovae
Chemical potentials
Stellar atmospheres
Voigt Function
Jeans escape
Polytropic stars
Cold white dwarfs
Hotter white dwarfs
Cold neutron stars
Stellar opacities
Neutrino energy loss rates
Ephemeris routines
FermiDirac functions
Galactic chemical evolution
Nuclear reaction networks
Nuclear statistical equilibrium
Laminar deflagrations
CJ detonations
ZND detonations
Fitting to conic sections
Unusual linear algebra
Derivatives on uneven grids
Pentadiagonal solver
Quadratics, Cubics, Quartics
Supernova light curves
Exact Riemann solutions
1D PPM Hydrodynamics
Verification problems
Plane  Cube Intersection
MESA
MESAWeb
FLASH
Zingale's software
Brown's dStar
GR1D code
Iliadis' STARLIB database
Herwig's NuGRID
Meyer's NetNuc
Presentations
Illustrations
Videos
Bicycle adventures
AAS Journals
2017 MESA Summer School
ASU+EdX AST111x
Teaching materials
Education and Public Outreach
2016 NSF SI2 PI Workshop
Contact: F.X.Timmes
my one page vitae,
full vitae,
research statement, and
teaching statement.


This instrument computes the state vectors for the sun, the nine
planets, the moon, the two martian satellites, four of the Galilean
satellites, eight of saturns moons, six of uranian moons, thousands of comets,
and half a million asteroids and other minor bodies.
See JPL
for the latest data files.
The values calculated compare
favorably with JPL
Horizons. A brief users guide is
in this README,
which is also included in the 117 MB
public_ephem.tbz bzip2 tarball
Xephem by Elwood
Downey is excellent, includes source code, and is a lot fun.
Starry Night is not free,
but a visually outstanding, particularily on openGL systems.
Both of these programs use the VSOP87 routines for the planetary state vectors;
neither deploy the JPL ephemeris files or the USNO vector astrometry toolkit
as used below.


The public_ephem.tbz bzip2 tarball contains five data files:
☊
unxp15502650.430  JPL DE430 unix littleendian binary file
for the sun, planets, and moon from +1550 to +2650.
If you want other binaries or want to to roll your own binary files, visit
JPL.
☊
comet_elements.dat  JPL osculatory orbital elements for comets.
Current as of 02Jan2016; get updated versions from
DATSCOM.
☊
numasteroids_elements.dat  JPL osculatory orbital elements for asteroids.
current as of 02Jan2016; get updated versions from
DATSCOM.
☊
ephem.e15  J2000 parameters for the Galilean satellites; from
Jay Lieske.
☊
redtass7.dat  time series arguments for eight of saturn's satellites;
from BDL.
Also check out the IERS site.


The public_ephem.tbz bzip2 tarball contains twelve library files:
☊
position_routine.f90  main that returns the state vector.
☊
ephem.dek  contains common block communications.
☊
initialize_routine.f90  initializations.
☊
jpl_routines.f90  customized version of the
JPL routines
that open, read, and interpolate the binary ephemeris files.
☊
novas_routines.f90  customized version of the USNO
NOVAS
routines.
☊
fxt_routines.f90  time and coordinate transforms, state vectors to orbital elements,
exact twobody solutions, and more.
☊
marsat_routines.f90  planetocentric state vectors of the martian satellites, from
ChaprontTouze 1990.
☊
lieske_routines.f90 
planetocentric state vectors of the jovian satellites, from
Lieske 1998.
☊
satsat_routines.f90 
planetocentric state vectors of saturn's satellites, from
Vienne & Duriez 1995.
☊
gust86_routines.f90 
planetocentric state vectors of the uranian satellites, from
Laskar & Jacobson 1987.
☊
glue.f90 
date and time from machine, string parsers, string to real converteds and more.
☊
trig_degrees.f90 
for compilers that don't support the circular functions in degrees.


The public_ephem.tbz bzip2 tarball contains nine applications:
☊
equinox.f90  dates of equinoxes and solstices.
☊
moon_phases.f90  times of the lunar phases.
flags conditions conducive for a potential lunar or solar eclipse.
☊
perihelion.f90  times of aphelions and perihelions.
Here are a few
periheleions and
apheleions for Earth.
☊
position.f90  state vectors in equatorial, ecliptic, and altazi coordinate systems
for geocentric, heliocentric or topographic centers.
☊
retrograde.f90  times of retrograde motion.
☊
rise.f90  rise, transit & set time of any object.
It uses a bombproof, but slower, search method.
☊
rise2.f90  rise, transit & set time of any object.
Using a fast iteration method, it can be fooled in unusual cases.
☊
solar_eclipse.f90  geographical track of a solar eclipse centerline,
reporting total, partial, annular, or noncentral phases.
☊
within.f90  dates when any two objects are within a given angular seperation.

